The orbit of Phi Cygni measured with long-baseline optical interferometry - Component masses and absolute magnitudes

Citations Over TimeTop 10% of 1992 papers

Abstract

view Abstract Citations (30) References (16) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Orbit of phi Cygni Measured With Long-Baseline Optical Interferometry: Component Masses and Absolute Magnitudes Armstrong, J. T. ; Hummel, C. A. ; Quirrenbach, A. ; Buscher, D. F. ; Mozurkewich, D. ; Vivekanand, M. ; Simon, R. S. ; Denison, C. S. ; Johnston, K. J. ; Pan, X. -P. ; Shao, M. ; Colavita, M. M. Abstract The orbit of the double-lined spectroscopic binary Phi Cygni, the distance to the system, and the masses and absolute magnitudes of its components are presented via measurements with the Mark III Optical Interferometer. On the basis of a reexamination of the spectroscopic data of Rach & Herbig (1961), the values and uncertainties are adopted for the period and the projected semimajor axes from the present fit to the spectroscopic data and the values of the remaining elements from the present fit to the Mark III data. The elements of the true orbit are derived, and the masses and absolute magnitudes of the components, and the distance to the system are calculated. Publication: The Astronomical Journal Pub Date: December 1992 DOI: 10.1086/116396 Bibcode: 1992AJ....104.2217A Keywords: Binary Stars; Speckle Interferometry; Stellar Magnitude; Stellar Mass; Stellar Orbits; Calibrating; Eccentricity; Orbital Elements; Stellar Spectrophotometry; Astronomy; BINARIES: SPECTROSCOPIC; INSTRUMENTS: INTERFEROMETERS full text sources ADS | data products SIMBAD (1)

Related Papers

• → Absolute magnitude calibration for red clump stars(2013)7 cited
• Determination of the mean absolute magnitude of RR Lyrae stars.(1972)
• Mean absolute magnitude of the RR Lyrae stars(1973)
• → Speckle Interferometry in Astrometry(1986)2 cited
• → Speckle Interferometry in Astrometry(1986)